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Updated: May 6, 2026

Setting Limits on Supersymmetry Using Simplified Models
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銀河の合併で多層のガス流入によって超大質量ブラックホールが直接形成される

L Mayer1, S Kazantzidis, A Escala

  • 1Institute for Theoretical Physics, University of Zürich, 190 Winterthurestrasse, Zürich 8057, Switzerland. lmayer@physik.unizh.ch

Nature
|August 27, 2010
PubMed
まとめ

巨大な原銀河の合併は,自然に超大質量ブラックホールを形成することができます. これらの合併は,直接的なガス崩壊の条件を作り出し,抑制された恒星形成の必要性を回避し,ブラックホールの急速な成長を可能にします.

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